where \(g_{\scriptscriptstyle N}=M(r)G/r^2\)  is the Newtonian acceleration,
and \(\nu \)  is the MOND interpolating function having the following behavior: In the high-acceleration, Newtonian regime, \(g_{\scriptscriptstyle N}\gg a_{0}\) , \(\nu (q\gg 1)\approx 1\) , and in the DML, we have \(\nu (q\ll 1)\approx q^{-1/2}\) . This functional dependence of \(g\)  on \(g_{\scriptscriptstyle N}\)  coincides with the original formulation of MOND in Ref. [1]}.
